November 6, 2003
09:00 AM (EST)

News Release Number: STScI-2003-31

Hubble Photographs Turbulent Neighborhood Near Eruptive Star

November 6, 2003: Dramatic dark dust knots and complex structures are sculpted by
the high-velocity stellar winds and high-energy radiation from
the ultra-luminous variable star called Eta Carinae. This image
shows a region in the Carina Nebula between two large clusters
of some of the most massive and hottest known stars. This NASA
Hubble Space Telescope close-up view shows only a three light-year-wide
portion of the entire Carina Nebula, which has a diameter of over
200 light-years. Taken with Hubble's Wide Field Planetary Camera 2
in July 2002, this color image is a composite of ultraviolet,
visible, and infrared filters that have been assigned the colors
blue, green, and red, respectively.

Q & A: Understanding the Discovery

1.
Where is the Carina Nebula?

The Carina Nebula, a naked-eye feature of the Southern Hemisphere
portion of the Milky Way, resides at a distance of 8,000 light-years.
The nebula has a diameter of over 200 light-years. This close-up
view is only a three light-year-wide portion of the entire nebula.

2.
What is the most massive star in the Carina Nebula?

The Carina Nebula contains the famous explosive variable star
Eta Carinae, or Eta Car. It contains as much mass as 100 suns,
and puts out more energy each second than 1 million suns. Eta
Car was one of the brightest stars in the sky for southern
observers in the 1800s, but it has since faded. It may continue
to experience future outbursts, which may increase its brightness
again at some point.

3.
What caused the structure seen in the Carina Nebula?

The filamentary structure visible in images of the Carina Nebula
is caused by turbulence in the circumstellar gas, which in turn
was caused by several stars shedding their outer layers. Cold
gas mixes with hot gas, leaving a veil of denser, opaque material
in the foreground. Dramatic dark dust knots and complex features
are sculpted by the high-velocity stellar winds and high-energy
radiation from massive and energetic stars in the nebula, such as
Eta Car.

4.
What happens to the material that is lost when a star erupts?

When massive stars like Eta Car shed their outer layers, the chemical
elements in the surrounding area create a potential reservoir for new
star formation. Many elephant-trunk shaped dust clouds are visible
throughout the Carina Nebula. These clouds may form into embryonic
solar systems.

5.
What do the colors in this image represent?

This color image is a composite of ultraviolet, visible, and
infrared filters that have been assigned the colors blue, green,
and red, respectively.

6.
Has Hubble imaged any other parts of the Carina Nebula?

A Hubble image of the Keyhole Nebula, also part of the Carina
Nebula, was taken in 1999. It shows similar structure, bright and
dark features, and is a direct result of massive stars, such as
Eta Car, interacting with their surroundings. The filters used to
image the Keyhole Nebula were ultraviolet, visible, and infrared,
as well as the emission filters oxygen, sulfur, and hydrogen. The
Keyhole Nebula image was released by the Hubble Heritage Project
in 2000.

7.
How can the Hubble telescope take more than one image at a time?

The Hubble telescope has several instruments that can be used
simultaneously to look at slightly different portions of the sky.
As one camera onboard Hubble takes data of an astronomical object,
another detector is able to take data of a nearby field at the
same time or "in parallel." Parallel observations with an unused
instrument during a programmed observation from another detector
is an extremely efficient use of Hubble's capabilities and allows
astronomers to probe parts of the sky that they would not otherwise
be able to investigate.